Morphological Corona 3 - 2017 Total Solar Eclipse

The solar corona is only visible for a few brief minutes during a total eclipse of the Sun.
Because the corona encompasses an enormous range of brightness (the innermost corona is over 1000 times brighter than the outer corona), it is difficult to capture an image that resembles what the eye sees.

It is a composite of images shot with two telescopes:
1) 57 separate exposures (1/2000 to 2 seconds) shot with an Astro-Physics 105EDT refractor and a Nikon D800 DSLR.
2) 38 separate exposures (1/2000 to 2 seconds) shot with a Vixen ED100sf refractor and a Nikon D810 DSLR.

The images were combined and processed using Photoshop CC 2017 and Photomatix Pro 6.
My PDF article "Digital Compositing Techniques for Coronal Imaging" is a bit dated (for example there is a discussion on digitizing negatives) but it still gives a useful description of some of the digital processing techniques I used to process my 2017 eclipse images.

There is a tremendous amount of structure visible in the underlying data, and much of it is revealed in this image.
A broader spatial filter has been used here to bring out some of the larger scale features present in the streamers.
This is done at the expense of exaggerating the more subtle details in the corona.
For an image processed to closely resemble the appearance of the corona as seen with the naked eye, see Visual Coronal 1A.

The Moon appears darker than the sky because of the huge contrast between the Moon's disk and the very bright inner corona adjacent to the Moon.
I've tried to preserve this visual impression in this image.

Note the bright star Regulus (Alpha Leo) to the far left of the corona.